The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar systemHarris, Joseph
History
The description and use of the globes and the orrery: To which is prefix'd, by way of introduction, a brief account of the solar system
Harris, Joseph
Astronomical models; Globes
In the foregoing problem, by the length of the day, we mean the time
from Sun-rising to Sun-set; and the night we reckoned from Sun-set,
’till he rose next morning. But it is found by experience, that _Total
Darkness_ does not commence in the evening, ’till the Sun has got 18
degrees below the horizon; and when he comes within the same distance
of the horizon next morning, we have the first _Dawn of Day_. This
faint light which we have in the morning and evening, before and after
the Sun’s rising and setting, is what we call the _Twilight_. [4]
Having rectified the globe for the latitude, the zenith, and the Sun’s
place, turn the globe and the quadrant of altitude until the Sun’s
place cuts 18 degrees below the horizon (if the quadrant reaches so
far) then the index upon the hour circle will shew the beginning or
ending of twilight after the same manner as before we found the time
of the Sun-rising and setting, in _Prob. 18_. But by reason of the
thickness of the wooden horizon, we can’t conveniently see, or compute
when the Sun’s place is brought to the point aforesaid. Wherefore the
globe being rectified as above directed, turn the globe, and also the
quadrant of altitude, Westward, until that point in the ecliptic, which
is opposite to the Sun’s place, cuts the quadrant in the 18th degree
above the horizon; then the hour index will shew the time when day
breaks in the morning. And if you turn the globe and the quadrant of
altitude, until the point opposite to the Sun’s place cuts the quadrant
in the Eastern hemisphere, the hour hand will shew when twilight ends
in the evening. Or, having found the time from midnight when the
morning twilight begins, if you reckon so many hours before midnight,
it will give the time when the evening twilight ends. Having found the
time when twilight begins in the morning, find the time of Sun-rising,
by _Prob. 18_, and the difference will be the duration of twilight.
Thus at _London_ on the 12th of _May_ twilight begins at three quarters
past one o’clock: The Sun rises at about half an hour past four: Whence
the duration of twilight now is 2¾ hours, both in the morning and
evening. On the 12th of _November_, the twilight begins at half an hour
past six, being somewhat above an hour before Sun-rising.
PROB. XXIV. _To find the time when total
Darkness ceases, or when the Twilight continues
from Sun-setting to Sun-setting, in any given
place._
Let the place be in the Northern hemisphere; then if the complement of
the latitude be greater than (the depression) 18 degrees, subtract 18
degrees from it, and the remainder will be the Sun’s declination North,
when total darkness ceases. But if the complement of the latitude is
less than 18 degrees, their difference will be the Sun’s declination
South, when the twilight begins to continue all night. If the latitude
is South, the only difference will be, that the Sun’s declination will
be on the contrary side.
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